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Masses of the $T_z=-3/2$ Nuclei $^{27}$P and $^{29}$S

Authors :
Fu, C. Y.
Zhang, Y. H.
Zhou, X. H.
Wang, M.
Litvinov, Yu. A.
Blaum, K.
Xu, H. S.
Xu, X.
Shuai, P.
Lam, Y. H.
Chen, R. J.
Yan, X. L.
Bao, T.
Chen, X. C.
Chen, H.
He, J. J.
Kubono, S.
Liu, D. W.
Mao, R. S.
Ma, X. W.
Sun, M. Z.
Tu, X. L.
Xing, Y. M.
Zhang, P.
Zeng, Q.
Zhou, X.
Zhan, W. L.
Litvinov, S.
Audi, G.
Uesaka, T.
Yamaguchi, Y.
Yamaguchi, T.
Ozawa, A.
Sun, B. H.
Sun, Y.
Xu, F. R.
Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Source :
Phys.Rev.C, Phys.Rev.C, 2018, 98 (1), pp.014315. ⟨10.1103/PhysRevC.98.014315⟩, Physical Review C, Physical Review C, American Physical Society, 2018, 98 (1), pp.014315. ⟨10.1103/PhysRevC.98.014315⟩
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

Isochronous mass spectrometry has been applied in the storage ring CSRe to measure the masses of the $T_z=-3/2$ nuclei $^{27}$P and $^{29}$S. The new mass excess value $ME$($^{29}$S) $=-3094(13)$~keV is 66(52)~keV larger than the result of the previous $^{32}$S($^3$He,$^{6}$He)$^{29}$S reaction measurement in 1973 and a factor of 3.8 more precise. The new result for $^{29}$S, together with those of the $T=3/2$ isobaric analog states (IAS) in $^{29}$P, $^{29}$Si, and $^{29}$Al, fit well into the quadratic form of the Isobaric Multiplet Mass Equation IMME. The mass excess of $^{27}$P has been remeasured to be $ME(^{27}$P$)=-685(42)$ keV. By analyzing the linear and quadratic coefficients of the IMME in the $T_z=-3/2$ $sd$-shell nuclei, it was found that the ratio of the Coulomb radius parameters is $R\approx0.96$ and is nearly the same for all $T=3/2$ isospin multiplets. Such a nearly constant $R$-value, apparently valid for the entire light mass region with $A>9$, can be used to set stringent constraints on the isovector and isotensor components of the isospin non-conserving forces in theoretical calculations.<br />7 pages, 4 figures

Details

Language :
English
ISSN :
24699985 and 24699993
Database :
OpenAIRE
Journal :
Phys.Rev.C, Phys.Rev.C, 2018, 98 (1), pp.014315. ⟨10.1103/PhysRevC.98.014315⟩, Physical Review C, Physical Review C, American Physical Society, 2018, 98 (1), pp.014315. ⟨10.1103/PhysRevC.98.014315⟩
Accession number :
edsair.doi.dedup.....84702ae4d32ad8c31a89b9626af8ba13